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      • KCI등재

        PANORAMIC VIEWS OF GALAXY CLUSTER EVOLUTION: GALAXY ECOLOGY

        Kodama, Tadayuki,Koyama, Yusei,Hayashi, Masao,Ken-ichi, Tadaki The Korean Astronomical Society 2010 天文學論叢 Vol.25 No.3

        Taking the great advantage of Subaru's wide field coverage both in the optical and in the near infrared, we have been providing panoramic views of distant clusters and their surrounding environments over the wide redshift range of 0:4 < z < 3. From our unique data sets, a consistent picture has been emerging that the star forming activity is once enhanced and then truncated in galaxy groups in the outskirts of clusters during the course of cluster assembly at z < 1. Such activity is shifted into cluster cores as we go further back in time to z ~ 1.5. At z = 2 - 2.5, we begin to enter the epoch when massive galaxies are actually forming in the cluster core. And by z ~ 3, we eventually go beyond the major epoch of massive galaxy formation. It is likely that the environmental dependence of star forming activity is at least partly due to the external environmental effects such as galaxy-galaxy interaction in medium density regions at z < 1, while the intrinsic effect of galaxy formation bias overtakes the external effect at higher redshifts, resulting in a large star formation activity in the cluster center.

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        Effect of leaf toughness and temperature on development in the lilac pyralid, Palpita nigropunctalis (Bremer) (Lepidoptera: Crambidae)

        Tetsuo Gotoh,Masao Koyama,Yuko Hagino,Kentaro Doke 한국응용곤충학회 2011 Journal of Asia-Pacific Entomology Vol.14 No.2

        This study focuses on three factors that affect the survival of the lilac pyralid, Palpita nigropunctalis (Lepidoptera:Crambidae): (1) the effect of leaf toughness on survival rate to clarify the availability of leaves as food, (2) the effect of temperature on immature development to determine the lower thermal threshold, and (3) the effect of temperature on head capsule width to clarify whether head capsule width can be used to discriminate among field-collected larval instars. Larvae could develop on Osmanthus fragrans var. aurantiacus leaves collected in April, but not on leaves collected in June or September which were too tough to eat. More than 80% of the larvae on the leaves of Ligustrum lucidum, Ligustrum japonicum, Ligustrum obtusifolium and Syringa vulgaris completed development, regardless of the collection time. P. nigropunctalis completed development on L. lucidum at temperatures from 15 to 27.5 °C with a photoperiod of either 15 L:9D or 16 L:8D,but not at 30 °C, at which temperature no eggs hatched. The lower thermal threshold and thermal constant for total development from egg to adult were estimated at about 7 °C and 450–460 degree-days. Most of the larvae were 5-instar type larvae (passed through 5 instars) regardless of the temperature, but a few 6-instar type larvae (4 of 355) were noted at temperatures of 22.5 °C and higher. No overlap of the ranges of head capsule widths was detected for the 5-instar type larvae, indicating that head capsule width can be used to discriminate among field-collected larval instars.

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